We study changes in the γ--ray intensity at very high energies observed from the γ--ray binary HESS J0632+057. Publicly available data collected by Cherenkov telescopes were examined by means of a simple method utilizing solely the number of source and background events. Our results point to time variability in signal from the selected object consistent with periodic modulation of the source intensity.
Cite
@article{arxiv.1409.5395,
title = {Time variability of the $\gamma$-ray binary HESS J0632+057},
author = {Stanislav Stefanik and Dalibor Nosek},
journal= {arXiv preprint arXiv:1409.5395},
year = {2014}
}